{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:4BA4GTAQOAFTWCJG5OHPAC6LI6","short_pith_number":"pith:4BA4GTAQ","schema_version":"1.0","canonical_sha256":"e041c34c10700b3b0926eb8ef00bcb47a3186082511b0b1dc9dbd5893bc1bbb1","source":{"kind":"arxiv","id":"1711.10726","version":1},"attestation_state":"computed","paper":{"title":"The SAMI Galaxy Survey: The Low-Redshift Stellar Mass Tully-Fisher Relation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. L. Schaefer, A. M. Hopkins, A. M. Medling, A. W. Green, B. Catinella, C. Tonini, F. DEugenio, H. Clark, I. S. Konstantopoulos, J. Bland-Hawthorn, J. J. Bryant, J. Lawrence, J.R. Callingham, J. T. Allen, J. V. Bloom, K. Glazebrook, L. Cortese, M. Goodwin, M. S. Owers, N. Lorente, N. Scott, R. E. McElroy, R. Sharp, S. M. Croom, S. N. Richards","submitted_at":"2017-11-29T08:41:11Z","abstract_excerpt":"We investigate the Tully-Fisher Relation (TFR) for a morphologically and kine- matically diverse sample of galaxies from the SAMI Galaxy Survey using 2 dimensional spatially resolved Halpha velocity maps and find a well defined relation across the stellar mass range of 8.0 < log(M*) < 11.5. We use an adaptation of kinemetry to parametrise the kinematic Halpha asymmetry of all galaxies in the sample, and find a correlation between scatter (i.e. residuals off the TFR) and asymmetry. This effect is pronounced at low stellar mass, corresponding to the inverse relationship between stellar mass and "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1711.10726","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-29T08:41:11Z","cross_cats_sorted":[],"title_canon_sha256":"2c2da86e007f15f3d6090935f0f4f7f93fe008963e5beec94a3e308bae683508","abstract_canon_sha256":"631e47786246b7a61152000fd693c72c3ca0ac46a7641d1183617b6eb8ef7968"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:51.397168Z","signature_b64":"Q2xujV81wY0aslAARWKliVEJrlnz+2Lp3OjXRovAmJkBXYeYzvQESOVELP4zNz9KnXefJpQlpoji1uaA0pSmCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e041c34c10700b3b0926eb8ef00bcb47a3186082511b0b1dc9dbd5893bc1bbb1","last_reissued_at":"2026-05-18T00:28:51.396501Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:51.396501Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The SAMI Galaxy Survey: The Low-Redshift Stellar Mass Tully-Fisher Relation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. L. Schaefer, A. M. Hopkins, A. M. Medling, A. W. Green, B. Catinella, C. Tonini, F. DEugenio, H. Clark, I. S. Konstantopoulos, J. Bland-Hawthorn, J. J. Bryant, J. Lawrence, J.R. Callingham, J. T. Allen, J. V. Bloom, K. Glazebrook, L. Cortese, M. Goodwin, M. S. Owers, N. Lorente, N. Scott, R. E. McElroy, R. Sharp, S. M. Croom, S. N. Richards","submitted_at":"2017-11-29T08:41:11Z","abstract_excerpt":"We investigate the Tully-Fisher Relation (TFR) for a morphologically and kine- matically diverse sample of galaxies from the SAMI Galaxy Survey using 2 dimensional spatially resolved Halpha velocity maps and find a well defined relation across the stellar mass range of 8.0 < log(M*) < 11.5. We use an adaptation of kinemetry to parametrise the kinematic Halpha asymmetry of all galaxies in the sample, and find a correlation between scatter (i.e. residuals off the TFR) and asymmetry. This effect is pronounced at low stellar mass, corresponding to the inverse relationship between stellar mass and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.10726","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1711.10726","created_at":"2026-05-18T00:28:51.396609+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.10726v1","created_at":"2026-05-18T00:28:51.396609+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.10726","created_at":"2026-05-18T00:28:51.396609+00:00"},{"alias_kind":"pith_short_12","alias_value":"4BA4GTAQOAFT","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"4BA4GTAQOAFTWCJG","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"4BA4GTAQ","created_at":"2026-05-18T12:30:58.224056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6","json":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6.json","graph_json":"https://pith.science/api/pith-number/4BA4GTAQOAFTWCJG5OHPAC6LI6/graph.json","events_json":"https://pith.science/api/pith-number/4BA4GTAQOAFTWCJG5OHPAC6LI6/events.json","paper":"https://pith.science/paper/4BA4GTAQ"},"agent_actions":{"view_html":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6","download_json":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6.json","view_paper":"https://pith.science/paper/4BA4GTAQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.10726&json=true","fetch_graph":"https://pith.science/api/pith-number/4BA4GTAQOAFTWCJG5OHPAC6LI6/graph.json","fetch_events":"https://pith.science/api/pith-number/4BA4GTAQOAFTWCJG5OHPAC6LI6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6/action/storage_attestation","attest_author":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6/action/author_attestation","sign_citation":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6/action/citation_signature","submit_replication":"https://pith.science/pith/4BA4GTAQOAFTWCJG5OHPAC6LI6/action/replication_record"}},"created_at":"2026-05-18T00:28:51.396609+00:00","updated_at":"2026-05-18T00:28:51.396609+00:00"}